Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

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  • Using the Hanle Effect in Mg II k to Quantify the Open Flux above the Solar Poles
    We test the use of the Mg II resonant lines for measurement of the magnetic field at the top of the chromosphere of polar coronal holes (CHs). The Hanle effect in the core of Mg II k enables access to a regime of field strengths where the Zeeman effect has little diagnostic value (especially at the solar poles, where most of the field is transverse
    Hofmann, Ryan A. et al.

    Fecha de publicación:

    9
    2025
    Número de citas
    0
  • Updated Masses for the Gas Giants in the Eight-planet Kepler-90 System Via Transit-timing Variation and Radial Velocity Observations
    The eight-planet Kepler-90 system exhibits the greatest multiplicity of planets found to date. All eight planets are transiting and were discovered in photometry from the NASA Kepler primary mission. The two outermost planets, g (P g = 211 days) and h (P h = 332 days), exhibit significant transit-timing variations (TTVs), but were only observed six
    Shaw, David E. et al.

    Fecha de publicación:

    9
    2025
    Número de citas
    1
  • The Tremaine-Weinberg method at high redshifts
    This paper examines the reliability of the Tremaine-Weinberg (TW) method in measuring the pattern speed of barred galaxies at high redshifts. Measuring pattern speeds at high redshift may help to shed light on the time evolution of interactions between galactic bars and dark matter halos. The TW method has been extensively employed for nearby
    Roshan, Mahmood et al.

    Fecha de publicación:

    9
    2025
    Número de citas
    1
  • The TESS Grand Unified Hot Jupiter Survey. III. Thirty More Giant Planets
    We present the discovery of 30 transiting giant planets that were initially detected using data from NASA's Transiting Exoplanet Survey Satellite mission. These new planets orbit relatively bright (G ≤ 12.5) FGK host stars with orbital periods between 1.6 and 8.2 days, and have radii between 0.9 and 1.7 Jupiter radii. We performed follow-up ground
    Yee, Samuel W. et al.

    Fecha de publicación:

    9
    2025
    Número de citas
    1
  • The star HIP 41378 potentially misaligned with its cohort of long-period planets
    The obliquity between the stellar spin axis and the planetary orbit, detected via the Rossiter-McLaughlin (RM) effect, is a tracer of the formation history of planetary systems. While obliquity measurements have been extensively applied to hot Jupiters and short-period planets, they remain rare for cold and long-period planets due to observational
    Grouffal, S. et al.

    Fecha de publicación:

    9
    2025
    Número de citas
    0
  • The spectral diversity of outer icy bodies revealed by JWST and its link to early Solar System processes
    Introduction:Small bodies in the trans-Neptunian region are key to understanding Solar System formation and evolution. Trans-Neptunian objects (TNOs) are relics of planetary formation in the outer protoplanetary disk, but most of them were later affected by the giant planet instability and the dynamical evolution of the Solar System, with the
    Brunetto, Rosario et al.

    Fecha de publicación:

    9
    2025
    Número de citas
    0